dc.creatorGONCALVES, Denise R.
dc.creatorMAGRINI, Laura
dc.creatorMUNARI, Ulisse
dc.creatorCORRADI, Romano L. M.
dc.creatorCOSTA, Roberto D. D.
dc.date.accessioned2012-10-20T02:12:03Z
dc.date.accessioned2018-07-04T15:29:50Z
dc.date.available2012-10-20T02:12:03Z
dc.date.available2018-07-04T15:29:50Z
dc.date.created2012-10-20T02:12:03Z
dc.date.issued2008
dc.identifierMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v.391, n.1, p.L84-L87, 2008
dc.identifier0035-8711
dc.identifierhttp://producao.usp.br/handle/BDPI/27014
dc.identifier10.1111/j.1745-3933.2008.00561.x
dc.identifierhttp://dx.doi.org/10.1111/j.1745-3933.2008.00561.x
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1623664
dc.description.abstractWe report the discovery of the first known symbiotic star in IC10, a starburst galaxy belonging to the Local Group, at a distance of similar to 750 kpc. The symbiotic star was identified during a survey of emission-line objects. It shines at V = 24.62 +/- 0.04, V - R(C) = 2.77 +/- 0.05 and R(C) - I(C) = 2.39 +/- 0.02, and suffers from E(B-V) = 0.85 +/- 0.05 reddening. The spectrum of the cool component well matches that of solar neighbourhood M8III giants. The observed emission lines belong to Balmer series, [S II], [N II] and [O III]. They suggest a low electronic density, negligible optical depth effects and 35 000 < T(eff) < 90 000 K for the ionizing source. The spectrum of the new symbiotic star in IC10 is an almost perfect copy of that of Hen 2-147, a well-known Galactic symbiotic star and Mira.
dc.languageeng
dc.publisherWILEY-BLACKWELL PUBLISHING, INC
dc.relationMonthly Notices of the Royal Astronomical Society
dc.rightsCopyright WILEY-BLACKWELL PUBLISHING, INC
dc.rightsrestrictedAccess
dc.subjectbinaries: symbiotic
dc.subjectgalaxies: individual: IC10
dc.subjectLocal Group
dc.titleDiscovery in IC10 of the farthest known symbiotic star
dc.typeArtículos de revistas


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